CWNU 154

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0.25 UTI
0.25
CN
0.3
Cdens
0.12
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.12 Very low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 154 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 77.869 38.13 0.882 -0.343 -2.147 -7.354
Zhang et al. 2024 77.942 38.105 – – – –
Hunt & Reffert 2024 77.942 38.105 0.892 -0.321 -2.179 -10.775
Cavallo et al. 2024 77.848 38.156 0.892 – – –
Hunt & Reffert 2023 77.942 38.105 0.892 -0.321 -2.179 -10.775
He et al. 2022 77.952 38.107 0.87 -0.34 -2.27 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 1.15 0.93 0.67 56 0.051 112 – –
Zhang et al. 2024 – – – – -0.261(1) – – –
Hunt & Reffert 2024 – – – – – 112(1) – –
Cavallo et al. 2024 1.15 0.93 – 56 0.130 – – –
Hunt & Reffert 2023 1.03 0.75 0.67 111 – – – –
He et al. 2022 1.29 1.26 – 40 0.051 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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